The homotopy type of a topological stack

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1 The homotopy type of a topological stack Johannes Ebert, Mathematisches Institut der Universität Bonn Beringstraße Bonn, Germany ebert@math.uni-bonn.de January 12, 2009 Abstract The notion of the homotopy type of a topological stack has been around in the literature for some time. The basic idea is that an atlas X X of a stack determines a topological groupoid X with object space X. The homotopy type of X should be the classifying space BX. The choice of an atlas is not part of the data of a stack and hence it is not immediately clear why this construction of a homotopy type is well-defined, let alone functorial. The purpose of this note is to give an elementary construction of such a homotopy-type functor. 1 Introduction The concept of a stack (which originated in algebraic geometry) plays an increasingly important role in geometric topology, see for example [2], [5], [3], [4]. In this note we show how a stack defines an object of homotopy theory. We assume that the reader is familiar with the terminology of stacks. Therefore we will not spell out the basic definitions here. A stack over the site Top of topological spaces is a lax sheaf of groupoids on the site of topological spaces; we refer the reader to the excellent [8] an explanation of this definition. Stacks over Top form a 2-category all of whose 2-morphisms are isomorphisms. There are several possible notions of topological stacks. Our notion is made explicit in 2.3. Essentially, a topological stack is a stack over Top which can be represented by a topological groupoid. Let TopStacks denote the 2-category of topological stacks. For any 2-category S, we denote the underlying ordinary category by the symbol τ 1 S. We would like to construct a functor Ho : τ 1 TopStacks Top which assigns to a stack its homotopy type. For set-theoretical reasons, we need to restrict to small subcategories of S TopStacks. This level of sophistication is certainly sufficient for all applications of our construction to concrete mathematical problems. Furthermore, it turns out that we need to restrict to stacks which admit a presentation by a paracompact groupoid (see below for details). This is a rather mild condition, which is satisfied by virtually all stacks of interest in geometric topology. In the sequel, we assume that S is a small 2-category and there is a fixed 2-functor J : S TopStacks such that all stacks in the image of this functor admit a presentation by a paracompact groupoid. The first main result of this note is Theorem 1.1. There exists a functor Ho : τ 1 S Top, which assigns to s Ob(S) a topological space Ho(X) which is homotopy equivalent to BX, when X is a groupoid presenting the topological X = J (s). If f,g are two 1-morphisms with the same source and target, then Ho(f) and Ho(g) are homotopic if f and g are 2-isomorphic or if J (f) and J (g) are concordant (see Definition 2.10 below). 1

2 Let π 0 (S) be the category which is obtained from τ 1 S by identification of 2-isomorphic 1- morphisms; there is a quotient functor τ 1 S π 0 (S). Note that the fully faithful Yoneda embedding st : Top TopStacks defines a fully faithful functor Top π 0 TopStacks - homotopic but different maps of spaces do not yield 2-isomorphic morphisms of stacks. Furthermore, let HoTop be the homotopy category of topological spaces. As a corollary of Theorem 1.1, we obtain the existence of a homotopy type functor π 0 (S) HoTop. This homotopy type functor extends both, the obvious functor Top HoTop and the functor from topological groups to HoTop sending G to BG. There is an essential feature of homotopy types which is abandoned in Theorem 1.1. Let us describe what is missing. Let X be a space. Then we denote, as usual, the stack st(x) by the symbol X; there is no danger of confusion. The space Ho(X) should come with a map η X : Ho(X) X which should be a universal weak equivalence, i.e. for any space Y and any Y X, the pullback Y X Ho(X) Y is a weak homotopy equivalence (the morphism Y X is automatically representable by [11], Corollary 7.3; thus Y X Ho(X) is a topological space). The map η X is a generalization of the map BG /G given by the universal principal G-bundle. Obviously, it is desirable that the maps η X assemble to a natural transformation η : st Ho τ 1 J of functors τ 1 S τ 1 TopStacks. We were not able to construct such a natural transformation on the nose, but only up to contractible choice and up to 2-isomorphism. The following two definition make these notions precise. Definition 1.2. Let C be a (discrete, small) category. A functor defined up to contractible choice is a triple ( C,p,F), where C is a topological category which has the same objects as C, p : C C is a functor which is the identity on objects and a weak homotopy equivalence on morphism spaces (i.e. C is a thickening of C in the sense that the morphisms in C are replaced by contractible spaces of morphisms) and F : C Top is a continuous functor. Definition 1.3. Let A be a topological category with discrete object set and B be a discrete 2- category all of whose 2-morphisms are isomorphisms. Let F 0,F 1 : A B be two functors. A pseudo-natural transformation η assigns to every object a A a 1-morphism η a : F 0 (a) F 1 (a) and to every morphism f : a a of A a 2-isomorphism η f : F 1 (f) η a η a F 0 (f) such that η ida = id ηa and such that for any pair f,f of composable morphisms, the 2-isomorphisms η f,η f and η f f are compatible. For most (but not all) constructions of homotopy theory, a functor defined up to contractible choice is as good as an honest functor. Therefore the following theorem should be a satisfactory result for many purposes. Theorem 1.4. Let S be as above. Then there exists a functor defined up to contractible choice ( τ 1 S,p, Ho). The functor Ho is related to the functor Ho p from Theorem 1.1 by a zig-zag of natural transformations which are weak homotopy equivalences on each object. Moreover, there exists a pseudo-natural transformation η : st Ho J p of functors τ 1 S TopStacks. For any stack X S, the morphism η X : Ho(X) X is a universal weak equivalence, in the sense that for any space Y and any Y X, the pullback Y X Ho(X) Y is a weak homotopy equivalence. The results of the present paper are very similar to those of Behrang Noohi s recent paper [12] (in fact, they are slightly weaker). Proposition 11.2 in [12] implies 1.4. On the other hand our treatment is more elementary. Therefore we claim that the present paper should be useful for anyone whose main interest is in the applications of topological stacks to problems in geometry. However, there is a flaw in the theory (also in [12]) which we will describe now. Given a homotopy invariant functor F from spaces to groups (or any other discrete category), we can extend F to stacks via ˆF(X) := F(Ho(X)). (1.5) 2

3 It follows that ˆF(η X ) is an isomorphism. For many of the functors of algebraic topology, including singular (co)homology or homotopy groups, this is a reasonable definition. But there are important homotopy-invariant functors on spaces for which 1.5 is not a good definition. The prime example is complex K-theory. Any reasonable definition of the K-theory of a stack should satisfy K 0 ( /G) = RG for a compact Lie group G (RG is the representation ring). In fact the definition of the K- theory of a stack given in [5] satisfies this condition. On the other hand, the celebrated Atiyah-Segal completion theorem [1] shows, among other things, that the natural map RG K 0 (BG) is not an isomorphism. It follows that, in the present setup, K-theory of a stack is not homotopy-invariant. Gepner and Henriques [6] developed a finer homotopy theory of stacks in which K-theory is homotopy invariant. On the other hand, their theory is much more involved than ours. Here is a brief outline of the paper. In section 2, we discuss the notion of a principal X-bundle for an arbitrary topological groupoid X and define the stack X 0 /X 1 of principal X-bundles, which is the prototype of a topological stack. Then we construct the universal principal X-bundle. The material in this section is a rather straightforward generalization of the classical theory of classifying spaces for topological groups. However, we need to be precise on the point-set level, and Theorem 2.7 is stronger than what is standard in the theory of fibre bundles. Section 3 contains the proofs of Theorem 1.1 and 1.4. In an appendix A, we show a technical result which guarantees the paracompactness of the classifying space of a paracompact groupoid. Acknowledgements The author was supported by a postdoctoral grant from the German Academic Exchange Service (DAAD). He enjoyed the hospitality of the Mathematical Institute of the University of Oxford. He is particularly grateful to Jeff Giansiracusa for numerous discussions about stacks. He also wants to thank the anonymous referee who pointed out a mistake at a crucial step of the argument in an earlier version of this paper. 2 Groupoids and stacks Principal bundles for groupoids Let X = (X 0, X 1,s,t,e,m,ι) be a topological groupoid: X 0 is the object space, X 1 the morphism space, s,t : X 1 X 0 are source and target maps, m : X 1 X0 X 1 X 1 is the multiplication, e : X 0 X 1 is the unit map and ι : X 1 X 1 sends a morphism to its inverse. The maps s,t,e,m,ι are continuous and satisfy the usual identities. We use the following convention: the product xy = m(x,y) of x,y X 1 is defined if (and only if) t(x) = s(y). We say that an X-space over a space X consists of a space E, two maps p : E X and q : E X 0 and an action α : E X0 X 1 = {(e,γ) E X 1 q(e) = s(γ)} E over X which is compatible with the projection to X and the multiplication in X. In other words, the diagrams E X0 X 1 α E (P 1 is the projection onto the first factor) and E p 1 p X p E X0 X 1 X0 X 1 (id,m) E X0 X 1 (α,id) E X0 X 1 α E α 3

4 are required to commute. Isomorphisms, pullbacks and restrictions of X-spaces over X are defined in the obvious way. We will often write an X-space shortly as p : E X, with the maps q and α understood. To define principal X-bundles, we start with trivial bundles. The diagram X 1 t X 0 (2.1) s X 0 defines an X-space over X 0 (p := s, q := t, α := m). This serves as the local model for a principal X-bundle. Definition 2.2. Let X be a topological groupoid and let X be a topological space. A principal X-bundle on X is an X-space (E;p,q,α) over X which is locally trivial in the sense that each x X has an open neighborhood U X which admits a map h : U X 0 and an isomorphism of the restriction E U with the pullback of 2.1 via h. There is an equivalent notion which is more abstract but also more common in the theory of stacks. It is the notion of X-torsors. We will not use this notion, but we explain it briefly. Given any map T X of spaces, we can form the groupoid X T with object space T and morphism space T X T. We say that a morphism of topological groupoids X Y is called cartesian if the diagrams X 1 Y 1 X 1 Y 1 s s X 0 Y 0 X 0 Y 0 are cartesian. An X-torsor on a space X is a map p : T X which admits local sections together with a cartesian morphism of groupoids φ : X T X. Given such an X-torsor, a principal X-bundle is given as follows: The total space E is just T and φ 0 gives a map E X 0. The action α is the composition T X0 X 1 = T X T T (projection onto the first factor). Conversely, let (E,p,q,α) be a principal X-bundle. Put T := E. The map p has local sections by the definition of a principal bundle 1. Let e 1,e 2 E be two points in the same fibre, p(e 1 ) = p(e 2 ), i.e. (e 1,e 2 ) E X E. There exists a unique γ (e1,e 2) X 1 such that α(e 1,γ (e1,e 2)) = e 2. Assigning (e 1,e 2 ) γ (e1,e 2) defines a map φ 1 : E X E X 1 which is continuous by the local triviality of a principal bundle. This map fits into a commutative diagram t t T X T φ X 1 T s,t which is easily seen to be cartesian. We will not use the concept of a torsor any more in this note. One can also describe principal X-bundles in terms of transition functions, see [7]. It is worth to spell out what a principal X-bundle is for familiar groupoids. Let Y be a space, considered as a groupoid X without nontrivial morphisms. Let (E, p, q, α) be a principal X-bundle on X. The maps in 2.1 are identities; thus p : E X is a homeomorphism; q p 1 is a map X Y, and under these identifications α is the canonical homeomorphism X X X X. Thus a principal bundle for the trivial groupoid is the same as a continuous map X Y. 1 Note that ι : X 0 X 1 is a section to the map s. q X 0, s,t 4

5 A similar situation is met when X = Y U is the groupoid associated to an open cover U of the space Y (see [13]). The map E X is then an open cover of X, q is a collection of locally defined maps to Y (in fact, to the elements of the original open cover). The map α is precisely the information that all these locally defined maps fit together to form a globally defined map X Y. If G is a topological group, considered as a groupoid with one object, then the notion of principal G-bundle from Definition 2.2 agrees with the traditional notion of a principal bundle, with the exception that we assume that G acts from the left on the total space. Similarly, if G acts on the space Y from the left, we form the groupoid G Y : the object space is Y, the morphism space is G Y and the action is used for the structural map of a groupoid. A principal G Y -bundle on a space X consists of a principal G-bundle P X and an G-equivariant map q : P Y. The stack of principal X-bundles The collection of all principal X-bundles on a space X, together with their isomorphisms, forms a groupoid which we denote by X 0 /X 1 (X). The functor X X 0 /X 1 (X) is a (lax) presheaf of groupoids on the site of topological spaces. The local nature of principal bundles shows that this is actually a sheaf of groupoids, in other words, a stack, which we denote by X 0 /X 1. Clearly, morphisms of groupoids yield morphisms of stacks and natural transformations of morphisms give 2-morphisms of stacks. Thus there is a 2-functor from topological groupoids to stacks, sending X to X 0 /X 1. This 2-functor is far from being an equivalence of categories. There can be a morphism φ : X Y of groupoids such that the induced morphism φ : X 0 /X 1 Y 0 /Y 1 is an equivalence, but φ does not have an inverse. This is not particularily exotic: given a topological group G and a principal G-bundle P X, then the obvious groupoid morphism G P X induces an equivalence of stacks P /G = X, but there is no inverse unless P is trivial. A similar situation is met when U is an open cover of the space X which defines a groupoid X U and an equivalence X U X. It is essential for the theory of stacks to allow for inverses of these morphisms. It may seem that the stacks X 0 /X 1 are quite special, but this is not the case. The data of a stack X, a space X and a representable map ϕ : X X determines a topological groupoid X. Namely, X 0 = X, X 1 = X X X; the structure maps for a groupoid are easy to find and the proof of the groupoid axioms is easy as well. Moreover, the map ϕ determines a morphism ˆϕ : X 0 /X 1 X of stacks. It is easy to see that ϕ is a chart (in the sense of [11], Def. 7.1) if and only if ˆϕ is an equivalence of stacks. Definition 2.3. A stack X over the site Top is a topological stack if there exists a topological groupoid X and an equivalence of stacks X 0 /X 1 X. This notion agrees with the notion of a pretopological stack defined in [11], Def The universal principal bundle We now want to define the universal principal X-bundle. The topological category X X is the category of arrows in X; more precisely, an object is an arrow γ : x y in X and a morphism from (γ : x y) to (γ : x y) is a morphism δ : x x with 2 δγ := m(δ,γ ) = γ; there is no morphism (γ : x y) (γ : x y ) if y y. There is a topology on X X induced from the topology on X and the functor p : X X X; p(γ : x y) = x, p(δ) = δ is continuous. Similarly, the functor ζ : X X X 0 (the trivial groupoid with object space X 0 ) which sends γ : x y to y is continuous. In this note we say that the classifying space of a topological category C is the thick geometric realization N C of the nerve N C of the category. The thick realization X of a simplicial space X is the space X := n 0 X n n /, 2 Sic; remember our convention about multiplication in a groupoid. 5

6 where is the equivalence relation generated by (ϕ x,t) (x,ϕ t) for any injective map ϕ in the simplex category. We apply the classifying space construction to the functors p and ζ and obtain a diagram B(X X) Bζ X 0 (2.4) BX Bp and, furthermore, a map B(X X) X0 X 1 B(X X) which is given by multiplication. We will abbreviate EX := B(X X). In the appendix, we shall describe two other convenient models for the spaces BX and EX. Proposition 2.5. The diagram 2.4 is a principal X-bundle. The proof is a straightforward generalization of Milnor s construction of classifying spaces for topological groups. It is given in [7] and also in [12]. The proofs uses a different description of the topological space BX. We say a few words about the latter point in the appendix. Proposition 2.6. There exists a section σ : X 0 EX of Bζ and a deformation retraction of EX onto σ(x 0 ) over X 0. Consequently, the space of sections of Bζ is contractible. Proof. Let σ : X 0 X X be the functor which sends x to id : x x. Clearly ζ σ = id and there is an evident natural transformation T : id X X σ ζ. The composition T σ is the identity transformation. So after realization, σ defines the desired section and T defines the deformation retraction. The well-known theorem that a continuous natural transformation between two functors of topological categories defines a homotopy between the maps on classifying spaces still holds if the geometric realization of the nerve is replaced by the thick geometric realization, except that we now get a contractible space of preferred homotopies instead of just one (combine the standard proof of the theorem in [13] with [14], Prop. A.1 (iii) and an explicit computation of N (0 1) ). Theorem 2.7. Let E univ B univ be a principal X-bundle such that the space of sections to the structure map q : E univ X 0 is contractible. Then for any principal X-bundle E X on a paracompact space X, the space of bundle morphisms E E univ is weakly contractible. In particular, this applies to the bundle EX constructed above. Proof. Let us begin with the trivial principal X-bundle X 1 X 0 from 2.1. It is easy to see that the space of bundle morphisms from X 1 X 0 to E univ B univ is homeomorphic to the space of sections s : X 0 E univ of q. Thus, by assumption, the space of bundle morphisms is contractible in this case. The same argument applies for a trivial principal bundle over a space different from X 0. To achieve the global statement, we apply a trick, which ought to be standard in the theory of fibre bundles. Let p : E X (plus the additional data) be a principal X-bundle. Choose an open covering (U i ) i I of X, so that E Ui is trivial. For any finite nonempty S I, let U S := i S U i. Clearly, E US is trivial as well. Let F S := map X (E US,E univ ) be the space of bundle maps from E US to E univ. We have seen that F S is weakly contractible. For any T S, there is a restriction map r T S : F T F S. Let S be the S 1-dimensional simplex { i S t ii R S i t i = 1;t i 0}. We now claim that we can choose maps c S : S F S whenever T S. This is done by induction on S, using the con- such that rs T c T = c S T tractibility of F S. 6

7 Finally, let (λ i ) i I be a locally finite partition of unity subordinate to (U i ). For any point x X, let S(x) I be the (finite) set of all i I with x supp(λ i ). The formula c(y) = c S(p(y)) ( λ i (p(y))i)(y) i S(p(y)) defines a global bundle morphism. This shows that the space F of bundle morphisms is nonempty. A straightforward version of the preceding reasoning shows a relative version of it: if A X is a cofibrant inclusion, then any bundle map E A E univ extends to X. Thus F is connected. A parameterized version of these arguments shows that for any compact K, map(k; F) is nonempty and connected. Thus F is weakly contractible. Proposition 2.8. The map ν X : BX X 0 /X 1 given by the principal X-bundle 2.4 is a universal weak equivalence. For the proof of 2.8, we shall need a little lemma. Lemma 2.9. Let f : Z Y be a map between topological spaces. Suppose that for any map p : U Y, the space of sections to f U : U Y Z U is weakly contractible. Then f is a homotopy equivalence. Proof. We only need that the space is nonempty when p = id Y and path-connected when p = f. The assumptions imply that there exists a section s : Y Z. We have to show that s f : Z Z is homotopic to the identity. The space of sections to the map f Z : Z Y Z Z; (z 1,z 2 ) z 1 is homeomorphic to the space of maps g : Z Z with f g = f. The maps id Z and s f both belong to that space and by assumption they are connected by a homotopy. Proof of Proposition 2.8. Let Y be a paracompact space and let P be a principal X-bundle on Y, which gives a map Y X 0 /X 1. We have to show that ν X;Y : Y X0 /X 1 BX Y is a weak homotopy equivalence. Note that the space of sections to ν X;Y can be identified with the space of bundle maps P EX, which is weakly contractible by Theorem 2.7. Likewise, let p : Z Y be any map and let Q := p P. The space of sections to Z X0 /X 1 BX = Z Y Y X0 /X 1 BX Z is homeomorphic to the space of bundle maps from Q to EX, which is again contractible. Therefore Lemma 2.9 can be applied. The classical theorem that for a topological group G, the set of isomorphism classes of principal G-bundles on a space Y is in bijective correspondance to the set of homotopy classes of maps Y BG admits a generalization. Definition Let X and Y be stacks. Let h i : X Y be two morphisms. A concordance between h 0 and h 1 is a triple (h,β 0,β 1 ), where h : X [0,1] Y and β i is a 2-isomorphism h i j i h for i = 0,1 (j i denotes the inclusion X = X {i} X [0,1]). Let X[Y ] be the set of concordance classes of elements in X(Y ). The following is an immediate consequence of Proposition 2.8. Corollary Let X be represented by the groupoid X. Then there is a natural bijection X[Y ] = [Y ;BX]. An appropriate relative version is also true; we leave this to the reader. The last thing we want to show in this section is that Proposition 2.8 actually characterizes EX and BX up to homotopy. Let X be a groupoid presenting the stack X. Let p : X X be a universal weak equivalence, which gives rise to a principal X-bundle E X. We have seen that the space of bundle maps E EX is contractible. Any such bundle map gives rise to a map X BX. This map is a homotopy equivalences, which follows immediately from 2.8 and from the 2-commutativity of the diagram BX X X. 7

8 Paracompact groupoids Later on, we shall need a technical result. Slightly differing from standard terminology, we say that a topological space X is paracompact if any open covering of X admits a subordinate locally finite partition of unity. If X is Hausdorff and paracompact in the usual sense (i.e. any covering admits a locally finite refinement), then X is paracompact in the present sense, see [10], p We say that a topological groupoid X is paracompact and Hausdorff if all spaces X n of the nerve are paracompact and Hausdorff. In general, the paracompactness of X 0 and X 1 does not imply the paracompactness of X. However, there are quite large classes of groupoids which are paracompact and Hausdorff. Examples of stacks which are presentable by paracompact and Hausdorff groupoids include 1. All differentiable stacks modeled on finite-dimensional manifolds 3 : If X is a manifold and X X a representable surjective submersion, then all fibred products X n = X X X X...X are manifolds and hence they are paracompact. 2. More generally, differentiable stacks modeled on Fréchet manifolds (under some countability conditions) 3. All topological stacks obtained by taking complex points of algebraic stacks (some finiteness condition is involved). 4. Quotient stacks X/G if G and X are metrizable 4. Proposition A.3 says that the classifying space BX = N X of a paracompact and Hausdorff groupoid is paracompact. This is discussed in the appendix. 3 Proof of the main results We shall first prove Theorem 1.4 and then 1.1. Let us set up notation. First of all, let S be a small 2-category and J : S TopStacks be a 2-functor, such that any stack in the image of J admits a presentation by a paracompact groupoid. To simplify notation, we assume that J is the inclusion of a small subcategory; the argument in the general case is the same. Stacks will be denoted by German letters X,Y,Z and they are tacitly assumed to be in S; likewise for morphisms and 2-morphisms. By the corresponding symbols X, Y, Z we will denote paracompact groupoids representing the stacks. For any stack in S we choose a presentation by a paracompact groupoid 5, denoted by ϕ X : X 0 /X 1 X. We can view ϕ 1 X as a principal X-bundle on the stack X, denoted by U X. In section 2, we constructed a map ν X : BX X 0 /X 1. We consider the composition η X = ϕ X ν X : BX X. Consider a morphism f : X Y of stacks. There is a diagram BX BY ν X X 0 /X 1 ν Y Y 0 /Y 1 X ϕ X f Y, ϕ Y and the vertical maps are universal weak equivalences by Proposition 2.8. The pullback η X f U Y is a principal Y-bundle on BX. Let E f be the space of bundle morphisms from η X f U Y to the 3 As usual, we assume manifolds to be second countable. 4 It seems unlikely that the paracompactness of both G and X implies the paracompactness of the translation groupoid, because the product of two paracompact spaces is in general not paracompact. 5 Here we need the axiom of choice, hence we use that S is small. 8

9 universal Y-bundle EY BY. By Proposition A.3 BX is paracompact and therefore, by Theorem 2.7, E f is weakly contractible. Thus we get a 2-commutative diagram E f BX ǫ f BY (3.1) X η X p 2 f Y, η Y in TopStacks; ǫ f is the evaluation map and p 2 denotes the projection onto the second factor. If f : X Y and g : Y Z are morphisms, then there is a composition map c g,f : E g E f E g f which makes the diagram E gf BX ǫ gf BZ c g,f id ǫ g E g E f BX id ǫ f E g BY commutative. The map c g,f arises in the following way. There is a specified map EY U Y of Y-bundles. Thus any element of E f defines a map η X f U Y η Y U Y of Y-bundles and therefore, after application of the morphism g of stacks, a map η X f g U Z η Y g U Z of Z-bundles, which can be composed with any element of E g. The collection of these maps is associative in the sense that c h g,f (c h,g id) = c h,g f (id c g,f ) : E h E g E f E h g f when h,g,f are composable morphisms. Also, id E id. Any 2-isomorphism φ : f g yields an isomorphism η X f U Y = η X g U Y and hence a homeomorphism φ : E g E f. Moreover, the diagram E g BX ǫ f BY (3.2) φ id E f BX ǫg BY is commutative. Now we define an topological category τ 1 S. It has the same objects as S (and the discrete topology on the object set). The morphism spaces are τ 1 S(X;Y) := S(X;Y) with the composition described above. The morphism spaces have contractible components (one for each 1-morphism in S). There is an obvious functor p : τ 1 S τ 1 (S). The classifying space construction determines a continuous functor Ho : τ 1 S Top, which sends a stack X to the space BX and which is the identity on morphism spaces. The universal weak equivalences η X assemble to a pseudo-natural transformation of functors η : st Ho J p of functors τ 1 S τ 1 TopStacks (use 3.1 to verify this). This finishes the proof of Theorem 1.4. Theorem 1.1 follows from Theorem 1.4 and a rectification procedure for homotopy-commutative diagrams which is proven in Nathalie Wahl s paper [15], following ideas of Dwyer, Kan and G. Segal. Roughly, she proves that a functor which is defined up to contractible choices can be strictified. More precisely, Proposition 2.1. of loc. cit can be reformulated as follows. E f 9

10 Proposition 3.3. [15] Let C be a discrete small 6 category and let ( C,p,F) be a functor to Top which is defined up to contractible choice. Then there exists a functor p F : C Top and a zigzag of natural transformations, which are weak homotopy equivalences on all objects, connecting p p F and F. To finish the proof of Theorem 1.1, take the functor Ho from Theorem 1.4 and put Ho(X) := p Ho(X). The additional assertions about 2-isomorphic and concordant morphisms of stacks follow from diagram 3.2 and 2.11, respectively. Uniqueness of the homotopy type functor So far, we have not addressed the question whether our construction is unique. Here is a uniqueness result which seems to be satisfactory enough. Let S be a small category of stacks, all of whose objects can be presented by paracompact groupoids. Let ( τ 1 S,p, Ho) be the homotopy type functor and η : st Ho J p be the natural transformation constructed in Theorem 1.4. Let ( τ 1 S,p, Ho ) be a functor τ 1 S Top, defined up to contractible choice and let η : st Ho J p be a natural transformation of functors such that η X is a universal weak equivalence for any object X of S. These two functors together yield a functor defined up to contractible choice on the category S {0,1}. Using the arguments from the proof of Theorem 1.4, one can easily show: Proposition 3.4. Under the circumstances above, there exists a functor Ho : S (0 1) Top, defined up to contractible choice which agrees with ( τ 1 S,p, Ho) on S {0} and with ( τ 1 S,p, Ho ) on S {1}. The natural transformations η and η yield a natural transformation. A Appendix: Point-set-topology of classifying spaces Let X be a topological groupoid. There are three different descriptions of the universal X-bundle each of which has some advantages. The first model, which was used in section 2 is the thick geometric realization of the categories X X and X. The use of this model makes the proofs of Lemma 2.6 and hence Theorem 2.7 particularly transparent. Another description goes back to Haefliger [7]; it is a generalization of Milnor s classical construction [9]. Let E Mil X be the space consisting of sequences (t 0 f 0,t 1 f 1,...), where f i X 1 all have the same target; t i [0,1], t i = 0 for all but finitely many i N, i t i = 1. Two sequences (t 0 f 0,t 1 f 1,...) and (t 0f 0,t 1f 1,...) are equivalent if t i = t i for each i and f i = f i whenever t i 0. The topology on E Mil X is the weakest topology such that the maps t i : E Mil X [0,1] and (0,1] X 1 are continuous. To obtain the space B Mil X, we divide by the following equivalence relation. Two sequences (t 0 f 0,t 1 f 1,...) and (t 0f 0,t 1f 1,...) are identified if t i = t i for each i and if there exists an f X 1 such that f i = f if for all i. A map E Mil X X 0 is defined by sending (t 0 f 0,t 1 f 1,...) to the common target of the f i s, and the action of X is equally easy to define. This description is convenient for the proof of Proposition 2.5, see [12]. f i : t 1 i Lemma A.1. [13] There are natural homeomorphisms N X = B Mil X and N X X = E Mil X. There is a slightly different description of N X which helps to show Proposition A.3 below. Let X be an arbitrary simplicial space. Let sk n X := k n X k k /. Then 6 This is an essential assumption. X = colim n sk n X 10

11 and furthermore sk n X is the pushout X n n sk n 1 X (A.2) X n n sk n X, where sk 1 X =. Thus, sk n X is the double mapping cylinder of a map X n X n n sk n 1 X. Therefore sk n X sk n+1 X is a neighborhood retract, as X n+1 n+1 is a neighborhood retract in X n+1 n+1. Proposition A.3. Let X be a simplicial topological space such that all X n are paracompact and Hausdorff. Then the thick realization X is paracompact (but not necessarily Hausdorff). A sketch of the proof of Proposition A.3 can be found in [6], p. 14. Here are the details. First note that X n n is paracompact by [10], p.223. Therefore, the proof of Lemma A.3 is accomplished by the following two lemmata. Lemma A.4. Let X be a paracompact Hausdorff space, A X be a closed neighborhood retract, Y a paracompact space and let f : X Y be a continuous map. Then X A Y is paracompact. Lemma A.5. Let Y be the colimit of the sequence Y 1 Y 2... Assume that Y n is paracompact and closed in Y ; assume that Y n Y n+1 is a neighborhood retract and assume that Y n+1 \ Y n is paracompact and Hausdorff. Then Y is paracompact. Proof of Lemma A.4. Denote the quotient map by q = q X qy : X Y X A Y. Let B X A Y be an open neighborhood of q(y ) with a retraction map by r : B Y. Let (U i ) i I be an open covering of X A Y. Let (µ k ) k K be a locally finite partition of unity on Y which is subordinate to q 1 Y (U i). Clearly, r µ k is a locally finite partition of unity on B, but it is not subordinate to (U i ) i I B. Because X is paracompact and Hausdorff, it is normal ([10], p. 94, 99) and therefore Urysohn s lemma applies to it. Namely, we can find a function c k : X [0,1] such that supp(c k ) q 1 X (U i(k)) and such that c k (a) = 1 if a A and µ k (f(a)) > 0. Define a function ν k : X A Y [0,1] by ν k = µ k on q(y ) and ν k = c k r µ k on q(x). Clearly, ν k is a locally finite family of functions and the function ν = ν k is equal to 1 on q(y ). On the other hand, the space Z := ν 1 [0, 2 3 ] is a closed subspace of the paracompact Hausdorff space X and therefore also paracompact. Then take a partition of unity subordinate to (Z U i ) i I and use a bump function b with b = 0 if ν 1 3 and b = 1 if ν 2 3 to glue both partitions of unity together. Proof of Lemma A.5. To simplify notation, we shall talk about locally finite families of nonnegative functions without mentioning their individual members. If f is a locally finite family of nonnegative functions, we denote the sum of its members by f and the support of f simply by supp(f). Let U be an open covering of Y. Any locally finite family f of nonnegative functions on Y n which is subordinate to U Y n admits an extension to a locally finite family of nonnegative functions on all of Y, subordinate to U. This follows from an iterated application of Urysohn s lemma, using the retraction maps. Nowstart with a partition of unity µ (1) on Y 1 which is subordinate to U Y 1. Extend it as above to a locally finite family on Y, also denoted µ (1). Then choose a subordinate locally finite family µ (2) on Y 2 whose support is contained in { µ (1) 1 2 } and which is equal to 1 on { µ (1) 1 4 }. The sum µ (1) + µ (2) is a locally finite family of functions which is subordinate to U and whose support contains Y 2. We repeat this process: Assume that locally finite families of nonnegative functions µ (1),...µ (n) on Y are chosen, such that the support of n k=1 µ (k) contains Y n. We can define a new locally finite family µ (n+1) with support contained in { n k=1 µ (k) 1 n+1 } and whose sum is equal to 1 on { µ (1) +...µ (n) 1 2(n+1) }. These conditions guarantee that the union n=1µ (n) of these 11

12 families of functions is locally finite and that the union of the supports covers Y. An obvious formula produces a partition of unity out of this family. References [1] M. Atiyah, G. Segal: Equivariant K-theory and completion. J. Differential Geometry 3 (1969) p [2] K. Behrend, G. Ginot, B. Noohi, P. Xu: String topology for stacks, preprint arxiv: [3] J. Ebert, J. Giansiracusa: Pontrjagin-Thom maps and the homology of the moduli stack of stable curves arxiv: [4] J. Ebert, J. Giansiracusa: On the homotopy type of the Deligne-Mumford compactification, Algebraic & Geometric Topology 8 (2008) [5] D. Freed, M. Hopkins, C. Teleman: Loop groups and twisted K-theory I, preprint, arxiv (2007). [6] D. Gepner, A. Henriques: Homotopy theory of orbispaces, preprint, arxiv (2007). [7] A. Haefliger: Homotopy and integrability, Manifolds - Amsterdam 1970, Springer Lecture Notes in Mathematics 197 (1971), p [8] J. Heinloth: Some notes on differentiable stacks, Mathematisches Institut, Seminars 2004/05, Universität Göttingen (2005), p [9] J. Milnor: Construction of universal bundles II, Ann. of Math. 63 (1956), p [10] J. Nagata: Modern general topology. Second edition. North-Holland Mathematical Library, 33. North-Holland Publishing Co., Amsterdam, (1985). [11] B. Noohi: Foundations of topological stacks I, preprint, arxiv (2005). [12] B. Noohi: Homotopy types of stacks, preprint, arxiv: [13] G. Segal: Classifying spaces and spectral sequences. Inst. Hautes Études Sci. Publ. Math. IHES, 34 (1968), p [14] G. Segal: Categories and cohomology theories. Topology 13 (1974), p [15] N. Wahl: Infinite loop space structure(s) on the stable mapping class group, Topology 43 (2004), p

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